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2. File:Blue star.svg - Wikipedia

   en.wikipedia.org/wiki/File:Blue_star.svg

   The following other wikis use this file: Usage on el.wikipedia.org Ιωνικός Νίκαιας (ποδόσφαιρο) Usage on fr.wikipedia.org

3. List of blue straggler stars - Wikipedia

   en.wikipedia.org/wiki/List_of_Blue_straggler_stars

   Stars Star system Median distance Stars in system Spectral type Apparent magnitude (V) Comments and references Hyades: 5 HD 27482: 151: 1: B8V: The Closest Blue Straggler star to Earth. HD 27130: 153: 1: B8V: Chi Tauri: 153: 1: B9.5V: 71 Tauri: 153: 1: B8V: HD 283579: 153: 1: B9.5V: Coma Star Cluster: 3 13 Comae Berenices: 260 ± 20: 1: A3 V: 5 ...

4. List of luminous blue variable stars - Wikipedia

   en.wikipedia.org/wiki/List_of_Luminous_Blue...

   Star system Nebula Median distance Stars in system Spectral type Apparent magnitude (V) Comments and references P Cygni (34 Cygni) 5251±180: 1: B1-2 Ia-0ep: 4.82: The closest luminous blue variable star to Earth V4029 Sagittarii (HD 168607) 6,000 1 B9Ia + 8.12 to 8.29 [4] [5] near the Omega Nebula: V905 Scorpii (HD 160529) 6,100 1 LBV 6.66 [4] [5]

5. Pistol Star - Wikipedia

   en.wikipedia.org/wiki/Pistol_Star

   The Pistol Star is an extremely luminous blue hypergiant star, one of the most luminous and massive known stars in the Milky Way. It is one of many massive young stars in the Quintuplet cluster in the Galactic Center region. The star owes its name to the shape of the Pistol Nebula, which it illuminates.

6. Blue straggler - Wikipedia

   en.wikipedia.org/wiki/Blue_straggler

   Sketch of Hertzsprung–Russell diagram of a globular cluster, showing blue stragglers. A blue straggler is a type of star that is more luminous and bluer than expected. . Typically identified in a stellar cluster, they have a higher effective temperature than the main sequence turnoff point for the cluster, where ordinary stars begin to evolve towards the red gi

7. Blue giant - Wikipedia

   en.wikipedia.org/wiki/Blue_giant

   These stars also evolve through the core helium burning stage at constant luminosity, first increasing in temperature then decreasing again as they move toward the AGB. However, at the blue end of the horizontal branch, it forms a "blue tail" of stars with lower luminosity, and occasionally a "blue hook" of even hotter stars. [7]